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Time Dilation


  
Figure: A ``light clock'' is constructed aboard a glass spaceship (reference frame O') as follows: the ``tick'' of the clock is defined by one half the time interval  t'  required for the light from a strobe light to traverse the width of the ship (a height h), bounce off a mirror and come back, a total distance of 2h. In the reference frame of a ground-based observer O (with respect to whom the ship is travelling at a velocity u), the light is emitted a distance  2ut  behind the place where it is detected a time  2t  later. Since the light has further to go in the O frame (a distance $\ell = \sqrt{h^2 + u^2t^2}$), but it travels at  c  in both frames,  t  must be longer than  t'. This effect is known as TIME DILATION.
\begin{figure}
\begin{center}\epsfysize 2.5in
\epsfbox{PS/light_clock.ps}\end{center} %
\end{figure}

Fig. 23.3 pictures a device used by R.P. Feynman, among others, to illustrate the phenomenon of TIME DILATION: a clock aboard a fast-moving vessel (even a normal clock) appears23.7 to run slower when observed from the ``rest frame'' -- the name we give to the reference frame arbitrarily chosen to be at rest. Now, if we choose to regard the ship's frame as ``at rest'' (as is the wont of those aboard) and the Earth as ``moving,'' a clock on Earth will appear to be running slowly when observed from the ship! Who is right? The correct answer is ``both,'' in utter disregard for common sense. This seems to create a logical paradox, which we will discuss momentarily. But first let's go beyond the qualitative statement, ``The clock runs slower,'' and ask how much slower.

For this we need only a little algebra and geometry; nevertheless, the derivation is perilous, so watch carefully. For O', the time interval described in Fig. 23.3 is simply

\begin{displaymath}t' \; = \; {h \over c}
\qquad \qquad \hbox{\rm so that} \qquad \qquad
h \; = \; ct'
\end{displaymath}

whereas for O the time interval is given by

\begin{displaymath}t \; = \; {\ell \over c}
\qquad \qquad \hbox{\rm where} \qquad \qquad
\ell^2 \; = \; h^2 \; + \; u^2 t^2
\end{displaymath}

by the Pythagorean theorem. Expanding the latter equation gives

\begin{displaymath}t \; = \; {\sqrt{ h^2 + u^2 t^2 } \over c}
\qquad \qquad \hbox{\rm or} \qquad \qquad
c^2 t^2 \; = \; h^2 \; + \; u^2 t^2
\end{displaymath}

which is not a solution yet because it does not relate  t  to  t'. We need to ``plug in''   h2 = c2 t'2  from earlier, to get

\begin{eqnarray*}c^2 t^2 &=& c^2 t'^2 \; + \; u^2 t^2 \cr
\hbox{\rm or} \qquad  . . . 
 . . . , t^2 \cr
\hbox{\rm or} \qquad
t^2 \, (1 - \beta^2) &=& t'^2
\end{eqnarray*}


where we have recalled the definition   $\beta \equiv u/c$. In one last step we obtain

\begin{displaymath}t \; = \; { t' \over \sqrt{ 1 - \beta^2 } }
\qquad \qquad \hbox{\rm or} \qquad \qquad
t \; = \; \gamma \; t'
\end{displaymath}

where  $\gamma$  is defined as before: $\gamma \equiv 1/\sqrt{1 - \beta^2}$.

This derivation is a little crude, but it shows where  $\gamma$  comes from.



 
next up previous
Next: The Twin Paradox Up: The Special Theory of Relativity Previous: Simultaneous for Whom?
Jess H. Brewer
1999-03-19